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Time-resolved spectroscopy and photometry of an M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in H$\alpha$ line during the non-white light flare

, , , , , , , , , , , , , , , , , and . (2020)cite arxiv:2009.14412Comment: 39 pages, 15 figures, supplementary table (CSV format); accepted for publication in PASJ.

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Impact of Stellar Superflares on Planetary Habitability, , , , , , , , , and 8 other author(s). (2019)cite arxiv:1906.06797Comment: 37 pages, 19 figures, 4 tables. Accepted for publication in The Astrophysical Journal (on June 16, 2019).Do Kepler superflare stars really include slowly-rotating Sun-like stars ? - Results using APO 3.5m telescope spectroscopic observations and Gaia-DR2 data -, , , , , , , , , and . (2019)cite arxiv:1904.00142Comment: 71 pages, 31 figures, 10 tables. Accepted for publication in The Astrophysical Journal (on March 29, 2019).Time-resolved spectroscopy and photometry of an M dwarf flare star YZ Canis Minoris with OISTER and TESS: Blue asymmetry in H$\alpha$ line during the non-white light flare, , , , , , , , , and 8 other author(s). (2020)cite arxiv:2009.14412Comment: 39 pages, 15 figures, supplementary table (CSV format); accepted for publication in PASJ.Statistical properties of superflares on solar-type stars with Kepler data, , , , , , , and . (Jul 31, 2016)arcesetc: ARC Echelle Spectrograph Exposure Time Calculator., , , , , , , , and . J. Open Source Softw., 4 (34): 1130 (2019)